Observations of star-forming regions by the current and upcoming generation of
submillimeter polarimeters will shed new light on the evolution of magnetic fields over the …

Linearly polarized emission from dust grains and molecular spectroscopy is an effective
probe of the magnetic field topology in the interstellar medium and molecular clouds. The …

We present a detailed overview of the science goals and predictions for the Prime-Cam
direct-detection camera–spectrometer being constructed by the CCAT-prime collaboration …

In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …

A full understanding of high-mass star formation requires the study of one of the most elusive
components of the energy balance in the interstellar medium: magnetic fields. We report …

The formation of stellar clusters dictates the pace at which galaxies evolve, and solving the
question of their formation will undoubtedly lead to a better understanding of the Universe as …

We present a study of the relative orientation between the magnetic field projected onto the
plane of sky (B⊥) on scales down to 0.4 pc, inferred from the polarized thermal emission of …

FEEDBACK is a SOFIA (Stratospheric Observatory for Infrared Astronomy) legacy program
dedicated to study the interaction of massive stars with their environment. It performs a …

We present new observations of the active star formation region NGC 1333 in the Perseus
molecular cloud complex from the James Clerk Maxwell Telescope B-Fields In Star-forming …

We present synthetic dust polarization maps of simulated molecular clouds with the goal to
systematically explore the origin of the relative orientation of the magnetic field () with …